Constraints on Ultra Heavy Dark Matter Properties from Dwarf Spheroidal Galaxies with LHAASO Observations

Zhen Cao,F. Aharonian,Q. An, Axikegu,Y. X. Bai,Y. W. Bao,D. Bastieri, X. J. Bi,Y. J. Bi,J. T. Cai,Q. Cao,W. Y. Cao,Zhe Cao, J. Chang,J. F. Chang, A. M. Chen, E. S. Chen, Liang Chen,Lin Chen,Long Chen,M. J. Chen,M. L. Chen,Q. H. Chen,S. H. Chen,S. Z. Chen,T. L. Chen,Y. Chen,N. Cheng,Y. D. Cheng, M. Y. Cui,S. W. Cui,X. H. Cui,Y. D. Cui, B. Z. Dai,H. L. Dai,Z. G. Dai, Danzengluobu,D. della Volpe,X. Q. Dong,K. K. Duan,J. H. Fan,Y. Z. Fan,J. Fang,K. Fang,C. F. Feng, L. Feng,S. H. Feng,X. T. Feng,Y. L. Feng,S. Gabici,B. Gao,C. D. Gao, L. Q. Gao,Q. Gao, W. Gao,W. K. Gao,M. M. Ge,L. S. Geng,G. Giacinti,G. H. Gong,Q. B. Gou,M. H. Gu, F. L. Guo,X. L. Guo, Y. Q. Guo,Y. Y. Guo,Y. A. Han, H. H. He,H. N. He, J. Y. He,X. B. He,Y. He,M. Heller,Y. K. Hor,B. W. Hou,C. Hou,X. Hou,H. B. Hu,Q. Hu,S. C. Hu,D. H. Huang, T. Q. Huang,W. J. Huang,X. T. Huang,X. Y. Huang,Y. Huang,Z. C. Huang,X. L. Ji,H. Y. Jia,K. Jia,K. Jiang,X. W. Jiang,Z. J. Jiang,M. Jin,M. M. Kang,T. Ke,D. Kuleshov,K. Kurinov, B. B. Li, Cheng Li,Cong Li,D. Li,F. Li,H. B. Li,H. C. Li,H. Y. Li, J. Li,Jian Li,Jie Li,K. Li, W. L. Li,W. L. Li, X. R. Li,Xin Li,Y. Z. Li,Zhe Li,Zhuo Li,E. W. Liang,Y. F. Liang,S. J. Lin,B. Liu,C. Liu, D. Liu,H. Liu,H. D. Liu, J. Liu,J. L. Liu,J. Y. Liu,M. Y. Liu,R. Y. Liu,S. M. Liu,W. Liu,Y. Liu,Y. N. Liu,R. Lu,Q. Luo,H. K. Lv,B. Q. Ma,L. L. Ma,X. H. Ma,J. R. Mao,Z. Min,W. Mitthumsiri,H. J. Mu,Y. C. Nan,A. Neronov,Z. W. Ou,B. Y. Pang,P. Pattarakijwanich,Z. Y. Pei, M. Y. Qi,Y. Q. Qi,B. Q. Qiao,J. J. Qin,D. Ruffolo,A. Saiz,D. Semikoz,C. Y. Shao,L. Shao,O. Shchegolev,X. D. Sheng,F. W. Shu,H. C. Song,Yu. V. Stenkin,V. Stepanov,Y. Su, Q. N. Sun,X. N. Sun,Z. B. Sun,P. H. T. Tam,Q. W. Tang,Z. B. Tang,W. W. Tian, C. Wang,C. B. Wang, G. W. Wang,H. G. Wang,H. H. Wang,J. C. Wang,K. Wang, L. P. Wang,L. Y. Wang,P. H. Wang,R. Wang,W. Wang,X. G. Wang,X. Y. Wang,Y. Wang,Y. D. Wang,Y. J. Wang,Z. H. Wang,Z. X. Wang,Zhen Wang,Zheng Wang,D. M. Wei, J. J. Wei,Y. J. Wei,T. Wen, C. Y. Wu,H. R. Wu,S. Wu,X. F. Wu,Y. S. Wu,S. Q. Xi, J. Xia,J. J. Xia,G. M. Xiang,D. X. Xiao,G. Xiao,G. G. Xin,Y. L. Xin,Y. Xing,Z. Xiong, D. L. Xu, R. F. Xu,R. X. Xu,W. L. Xu,L. Xue,D. H. Yan,J. Z. Yan,T. Yan, C. W. Yang, F. Yang,F. F. Yang,H. W. Yang, J. Y. Yang,L. L. Yang,M. J. Yang,R. Z. Yang,S. B. Yang,Y. H. Yao,Z. G. Yao,Y. M. Ye,L. Q. Yin,N. Yin,X. H. You,Z. Y. You,Y. H. Yu,Q. Yuan,H. Yue,H. D. Zeng,T. X. Zeng,W. Zeng,M. Zha, B. B. Zhang, F. Zhang, H. M. Zhang,H. Y. Zhang, J. L. Zhang,L. X. Zhang,Li Zhang,P. F. Zhang,P. P. Zhang, R. Zhang,S. B. Zhang,S. R. Zhang,S. S. Zhang,X. Zhang,X. P. Zhang,Y. F. Zhang,Yi Zhang,Yong Zhang,B. Zhao,J. Zhao, L. Zhao,L. Z. Zhao,S. P. Zhao,F. Zheng,B. Zhou,H. Zhou,J. N. Zhou, M. Zhou,P. Zhou,R. Zhou,X. X. Zhou,C. G. Zhu,F. R. Zhu,H. Zhu,K. J. Zhu,X. Zuo

arxiv（2024）

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Abstract

In this work we try to search for signals generated by ultra-heavy dark matter at the Large High Altitude Air Shower Observatory (LHAASO) data. We look for possible gamma-ray by dark matter annihilation or decay from 16 dwarf spheroidal galaxies in the field of view of LHAASO. Dwarf spheroidal galaxies are among the most promising targets for indirect detection of dark matter which have low fluxes of astrophysical γ-ray background while large amount of dark matter. By analyzing more than 700 days observational data at LHAASO, no significant dark matter signal from 1 TeV to 1 EeV is detected. Accordingly we derive the most stringent constraints on the ultra-heavy dark matter annihilation cross-section up to EeV. The constraints on the lifetime of dark matter in decay mode are also derived.

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